Follow NASA’s Artemis I Moon Mission: Live Tracker, Latest Images, And Videos

Follow NASA’s Artemis I Moon Mission: Live Tracker, Latest Images, and Videos

On Nov. 16, 2022, the Artemis I mission officially began with the launch of the Orion spacecraft atop the Space Launch System rocket. The rocket and spacecraft lifted off from historic Launch Complex 39B at NASA’s Kennedy Space Center in Florida.

Now, the Orion spacecraft is about halfway through its journey around the Moon. Although the spacecraft is uncrewed, the Artemis I mission prepares us for future missions with astronauts, starting with Artemis II.

Stay up-to-date with the mission with the latest full-resolution images, mission updates, on-demand and live video.

A cross-section of the white, cylindrical Orion spacecraft dominates the left side of the screen. A rectangular solar array snaked with multicolored wires extends up and out to 2 o'clock, and four bell-shaped auxiliary thrusters point down from the body of the spacecraft. The small crescent Moon is isolated in the black of space in the distance beyond and below the solar array. Credit: NASA

Imagery:

Find full-resolution images from the Orion spacecraft as they are released here.

Launch imagery can be found here. When Orion splashes down in the Pacific Ocean on Dec. 11, the images will be available here, as well!

Videos:

This playlist contains informational videos, as well as upcoming and past live events, about Artemis I.

You can watch a livestream of the Artemis I mission here. (Just a note: the livestream may cut off during moments when the Orion team needs higher bandwidth for activities.)

Keep yourself updated on the upcoming broadcasts of Artemis milestones with the NASA TV schedule.

An animation shows the Orion spacecraft flying in space with the Moon in the far distance in the left side of the image. The text on the image reads:
Mission Time: 9 days, 7 hrs, 56 min
Orion is 233,784 miles from Earth, 57,639 miles from the Moon, cruising at 2,420 miles per hour.
P: (40690, -207007, -109608)
V: (2411, -52, -200)
O: 285º, 143.7º, 134.4º

Trackers:

Our Artemis I Tracker shows where the Orion spacecraft is along the trajectory of the mission.

“Eyes on the Solar System” shows where Orion is in relation to other NASA spacecraft and objects in the solar system:

“DSN Now” shows which antenna on Earth’s Deep Space Network is communicating with Orion.

Updates:

Read up on where Orion is and what’s next in the Artemis I mission with the Mission Blog.

Thank you so much for following with us on this historic mission. Go Artemis!

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Brings back childhood memories of studying NASA concept art for my Space Lego projects

Behold—the space station of the future! (…from 1973)

An artist's concept illustrating a cutaway view of the Skylab 1 Orbital Workshop (OWS). The OWS is a circular space with several vertical layers with floors that look like golden honeycombs. Different parts of the workshop are labeled, like the control and display panel where an astronaut in an orange jumpsuit works, film vaults, experiment support system, and the shower. Credit: NASA

This artist’s concept gives a cutaway view of the Skylab orbital workshop, which launched 50 years ago on May 14, 1973. Established in 1970, the Skylab Program's goals were to enrich our scientific knowledge of Earth, the sun, the stars, and cosmic space; to study the effects of weightlessness on living organisms; to study the effects of the processing and manufacturing of materials in the absence of gravity; and to conduct Earth-resource observations.

Three crews visited Skylab and carried out 270 scientific and technical investigations in the fields of physics, astronomy, and biological sciences. They also proved that humans could live and work in outer space for extended periods of time, laying the groundwork for the International Space Station.

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2 years ago

Rockets, Racecars, and the Physics of Going Fast

The SLS rocket and Orion spacecraft launch off Launch Pad 39B at NASA’s Kennedy Space Center on November 16, 2022, beginning the Artemis I mission. The ignition from the rocket’s two boosters and four engines lights up the night sky. Smoke is seen building up from the ground as the rocket takes flight. Image credit:  NASA/Joel Kowsky

When our Space Launch System (SLS) rocket launches the Artemis missions to the Moon, it can have a top speed of more than six miles per second. Rockets and racecars are designed with speed in mind to accomplish their missions—but there’s more to speed than just engines and fuel. Learn more about the physics of going fast:

The SLS rocket and Orion spacecraft launch from the launch pad at NASA’s Kennedy Space Center on November 16, 2022, beginning the Artemis I mission. This is a close-up view of the solid rocket boosters and RS-25 engines ignited for flight. Image credit:  NASA/Joel Kowsky

Take a look under the hood, so to speak, of our SLS mega Moon rocket and you’ll find that each of its four RS-25 engines have high-pressure turbopumps that generate a combined 94,400 horsepower per engine. All that horsepower creates more than 2 million pounds of thrust to help launch our four Artemis astronauts inside the Orion spacecraft beyond Earth orbit and onward to the Moon. How does that horsepower compare to a racecar? World champion racecars can generate more than 1,000 horsepower as they speed around the track.

This GIF shows the four RS_25 engines on the SLS rocket igniting one by one as they prepare to launch Artemis I. A red glow comes from below the engines as they ignite. Image credit: NASA

As these vehicles start their engines, a series of special machinery is moving and grooving inside those engines. Turbo engines in racecars work at up to 15,000 rotations per minute, aka rpm. The turbopumps on the RS-25 engines rotate at a staggering 37,000 rpm. SLS’s RS-25 engines will burn for approximately eight minutes, while racecar engines generally run for 1 ½-3 hours during a race.

NASA engineers test a model of the Space Launch System rocket in a wind tunnel at NASA’s Langley Research Center. The image is taken from a test camera. Image credit: NASA

To use that power effectively, both rockets and racecars are designed to slice through the air as efficiently as possible.

While rockets want to eliminate as much drag as possible, racecars carefully use the air they’re slicing through to keep them pinned to the track and speed around corners faster. This phenomenon is called downforce.

This GIF shows a full-scale solid rocket booster being tested at Northrop Grumman’s facility in Utah. The booster, laying horizontal, ignites and fires. Image credit: Northrop Grumman

Steering these mighty machines is a delicate process that involves complex mechanics.

Most racecars use a rack-and-pinion system to convert the turn of a steering wheel to precisely point the front tires in the right direction. While SLS doesn’t have a steering wheel, its powerful engines and solid rocket boosters do have nozzles that gimbal, or move, to better direct the force of the thrust during launch and flight.

Members of the Artemis I launch control team monitor data at their consoles inside the Launch Control Center at NASA’s Kennedy Space Center during the first launch attempt countdown on August 29. Image credit: NASA/Kim Shiflett

Racecar drivers and astronauts are laser focused, keeping their sights set on the destination. Pit crews and launch control teams both analyze data from numerous sensors and computers to guide them to the finish line. In the case of our mighty SLS rocket, its 212-foot-tall core stage has nearly 1,000 sensors to help fly, track, and guide the rocket on the right trajectory and at the right speed. That same data is relayed to launch teams on the ground in real time. Like SLS, world-champion racecars use hundreds of sensors to help drivers and teams manage the race and perform at peak levels.

Rockets, Racecars, And The Physics Of Going Fast

Knowing how to best use, manage, and battle the physics of going fast, is critical in that final lap. You can learn more about rockets and racecars here.

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2 years ago

Adobe steals your color

Adobe Steals Your Color

When a company breaks a product you rely on — wrecking decades of work — it’s natural to feel fury. Companies know this, so they try to deflect your rage by blaming their suppliers. Sometimes, it’s suppliers who are at fault — but other times, there is plenty of blame to go around.

For example, when Apple deleted all the working VPNs from its Chinese App Store and backdoored its Chinese cloud servers, it blamed the Chinese government. But the Chinese state knew that Apple had locked its devices so that its Chinese customers couldn’t install third-party apps.

That meant that an order to remove working VPNs and apps that used offshore clouds from the App Store would lock Apple customers into Chinese state surveillance. The order to block privacy tools was a completely foreseeable consequence of Apple’s locked-down “ecosystem.”

https://locusmag.com/2021/01/cory-doctorow-neofeudalism-and-the-digital-manor/

In 2013, Adobe started to shift its customers to the cloud, replacing apps like Photoshop and Illustrator with “Software as a Service” (“SaaS”) versions that you would have to pay rent on, every month, month after month, forever. It’s not hard to understand why this was an attractive proposition for Adobe!

Adobe, of course, billed its SaaS system as good for its customers — rather than paying thousands of dollars for its software up front, you could pay a few dollars (anywhere from $10-$50) every month instead. Eventually, of course, you’d end up paying more, assuming these were your professional tools, which you expected to use for the rest of your life.

For people who work in prepress, a key part of their Adobe tools is integration with Pantone. Pantone is a system for specifying color-matching. A Pantone number corresponds to a specific tint that’s either made by mixing the four standard print colors (cyan, magenta, yellow and black, AKA “CMYK”), or by applying a “spot” color. Spot colors are added to print jobs after the normal CMYK passes — if you want a stripe of metallic gold or a blob of hot pink, you specify its Pantone number and the printer loads up a separate ink and runs your media through its printer one more time.

Pantone wants to license this system out, so it needs some kind of copyrightable element. There aren’t many of these in the Pantone system! There’s the trademark, but that’s a very thin barrier. Trademark has a broad “nominative use” exception: it’s not a trademark violation to say, “Pantone 448C corresponds to the hex color #4a412a.”

Perhaps there’s a copyright? Well yes, there’s a “thin” database copyright on the Pantone values and their ink equivalents. Anyone selling a RIP or printer that translates Pantone numbers to inks almost certainly has to license Pantone’s copyright there. And if you wanted to make an image-editing program that conveyed the ink data to a printer, you’d best take a license.

All of this is suddenly relevant because it appears that things have broken down between Adobe and Pantone. Rather than getting Pantone support bundled in with your Adobe apps, you must now pay $21/month for a Pantone plugin.

https://twitter.com/funwithstuff/status/1585850262656143360

Remember, Adobe’s apps have moved to the cloud. Any change that Adobe makes in its central servers ripples out to every Adobe user in the world instantaneously. If Adobe makes a change to its apps that you don’t like, you can’t just run an older version. SaaS vendors like to boast that with cloud-based apps, “you’re always running the latest version!”

The next version of Adobe’s apps will require you to pay that $21/month Pantone fee, or any Pantone-defined colors in your images will render as black. That’s true whether you created the file last week or 20 years ago.

Doubtless, Adobe will blame Pantone for this, and it’s true that Pantone’s greed is the root cause here. But this is an utterly foreseeable result of Adobe’s SaaS strategy. If Adobe’s customers were all running their apps locally, a move like this on Pantone’s part would simply cause every affected customer to run older versions of Adobe apps. Adobe wouldn’t be able to sell any upgrades and Pantone wouldn’t get any license fees.

But because Adobe is in the cloud, its customers don’t have that option. Adobe doesn’t have to have its users’ backs because if it caves to Pantone, users will still have to rent its software every month, and because that is the “latest version,” those users will also have to rent the Pantone plugin every month — forever.

What’s more, while there may not be any licensable copyright in a file that simply says, “Color this pixel with Pantone 448C” (provided the program doesn’t contain ink-mix descriptions), Adobe’s other products — its RIPs and Postscript engines — do depend on licensable elements of Pantone, so the company can’t afford to tell Pantone to go pound sand.

Like the Chinese government coming after Apple because they knew that any change that Apple made to its service would override its customers’ choices, Pantone came after Adobe because they knew that SaaS insulated Adobe from its customers’ wrath.

Adobe customers can’t even switch to its main rival, Figma. Adobe’s just dropped $20b to acquire that company and ensure that its customers can’t punish it for selling out by changing vendors.

Pantone started out as a tech company: a way to reliably specify ink mixes in different prepress houses and print shops. Today, it’s an “IP” company, where “IP” means “any law or policy that allows me to control the conduct of my customers, critics or competitors.”

https://locusmag.com/2020/09/cory-doctorow-ip/

That’s likewise true of Adobe. The move to SaaS is best understood as a means to exert control over Adobe’s customers and competitors. Combined with anti-competitive killer acquisitions that gobble up any rival that manages to escape this control, and you have a hostage situation that other IP companies like Pantone can exploit.

A decade or so ago, Ginger Coons created Open Colour Standard, an attempt to make an interoperable alternative to Pantone. Alas, it seems dormant today:

http://adaptstudio.ca/ocs/

Owning colors is a terrible idea and technically, it’s not possible to do so. Neither UPS Brown nor John Deere Green are “owned” in any meaningful sense, but the companies certainly want you to believe that they are. Inspired by them and Pantone, people with IP brain-worms keep trying to turn colors into property:

https://onezero.medium.com/crypto-copyright-bdf24f48bf99

The law is clear that colors aren’t property, but by combining SaaS, copyright, trademark, and other tech and policies, it is becoming increasingly likely that some corporation will stealing the colors out from under our very eyes.

[Image ID: A Pantone swatchbook; it slowly fades to grey, then to black.]

2 years ago

12 Great Gifts from Astronomy

This is a season where our thoughts turn to others and many exchange gifts with friends and family. For astronomers, our universe is the gift that keeps on giving. We’ve learned so much about it, but every question we answer leads to new things we want to know. Stars, galaxies, planets, black holes … there are endless wonders to study.

In honor of this time of year, let’s count our way through some of our favorite gifts from astronomy.

Our first astronomical gift is … one planet Earth

So far, there is only one planet that we’ve found that has everything needed to support life as we know it — Earth. Even though we’ve discovered over 5,200 planets outside our solar system, none are quite like home. But the search continues with the help of missions like our Transiting Exoplanet Survey Satellite (TESS). And even you (yes, you!) can help in the search with citizen science programs like Planet Hunters TESS and Backyard Worlds.

This animated visualization depicts Earth rotating in front of a black background. Land in shades of tan and green lay among vast blue oceans, with white clouds swirling in the atmosphere. The image is watermarked with the text “Credit: NASA/Goddard Space Flight Center Scientific Visualization Studio” and “visualization.”

Our second astronomical gift is … two giant bubbles

Astronomers found out that our Milky Way galaxy is blowing bubbles — two of them! Each bubble is about 25,000 light-years tall and glows in gamma rays. Scientists using data from our Fermi Gamma-ray Space Telescope discovered these structures in 2010, and we're still learning about them.

This image captures the majestic “Fermi bubbles” that extend above and below our Milky Way galaxy, set against the black background of space. A glowing blue line horizontally crosses the center of the image, showing our perspective from Earth of our galaxy’s spiral arms and the wispy clouds of material above and below it. Cloudy bubbles, colored deep magenta to represent Fermi’s gamma-ray vision, extend above and below the galactic plane. These bubbles are enormous, extending roughly half of the Milky Way's diameter and filling much of the top and bottom of the image. The image is watermarked “Credit: NASA/DOE/Fermi LAT Collaboration.”

Our third astronomical gift is … three types of black holes

Most black holes fit into two size categories: stellar-mass goes up to hundreds of Suns, and supermassive starts at hundreds of thousands of Suns. But what happens between those two? Where are the midsize ones? With the help of NASA’s Hubble Space Telescope, scientists found the best evidence yet for that third, in between type that we call intermediate-mass black holes. The masses of these black holes should range from around a hundred to hundreds of thousands of times the Sun’s mass. The hunt continues for these elusive black holes.

This cartoon depicts two black holes as birds, with a small one representing a stellar-mass black hole on the left and an enormous one representing a supermassive black hole on the right. These two birds appear on a tan background and flap their wings, and then a circle with three question marks pops up between them to represent the intermediate-mass black holes that scientists are hunting for. The image is watermarked “Credit: NASA’s Goddard Space Flight Center.”

Our fourth and fifth astronomical gifts are … Stephan’s Quintet

When looking at this stunning image of Stephan’s Quintet from our James Webb Space Telescope, it seems like five galaxies are hanging around one another — but did you know that one of the galaxies is much closer than the others? Four of the five galaxies are hanging out together about 290 million light-years away, but the fifth and leftmost galaxy in the image below — called NGC 7320 — is actually closer to Earth at just 40 million light-years away.

A group of five galaxies that appear close to each other in the sky: two in the middle, one toward the top, one to the upper left, and one toward the bottom. Four of the five appear to be touching. One is somewhat separated. In the image, the galaxies are large relative to the hundreds of much smaller (more distant) galaxies in the background. All five galaxies have bright white cores. Each has a slightly different size, shape, structure, and coloring. Scattered across the image, in front of the galaxies are a number of foreground stars with diffraction spikes: bright white points, each with eight bright lines radiating out from the center. The image is watermarked with the text “Credits: NASA, ESA, CSA, and STScI.”

Our sixth astronomical gift is … an eclipsing six-star system

Astronomers found a six-star system where all of the stars undergo eclipses, using data from our TESS mission, a supercomputer, and automated eclipse-identifying software. The system, called TYC 7037-89-1, is located 1,900 light-years away in the constellation Eridanus and the first of its kind we’ve found.

This diagram shows the sextuple star system TYC 7037-89-1, a group of six stars that interact with each other in complex orbits. The stars are arranged in pairs: System A, System B, and System C, each of which is shown as having one larger white star and one smaller yellow star. The two stars of System A, in the upper left, are connected by a red oval and labeled "1.3-day orbit." The two stars of System C, just below System A, are connected by a turquoise oval and labeled "1.6-day orbit." Additionally, these two systems orbit each other, shown as a larger blue oval connecting the two and labeled "A and C orbit every 4 years." On the other side of the image, in the bottom right, the two stars of System B are connected by a green oval and labeled "8.2-day orbit." Lastly, Systems A, B and C all interact with System B orbiting the combined A-C system, shown as a very large lilac oval labeled "AC and B orbit every 2,000 years." A caption at the bottom of the image notes, "Star sizes are to scale, orbits are not." The image is watermarked with the text “Illustration” and “Credit: NASA's Goddard Space Flight Center.”

Our seventh astronomical gift is … seven Earth-sized planets

In 2017, our now-retired Spitzer Space Telescope helped find seven Earth-size planets around TRAPPIST-1. It remains the largest batch of Earth-size worlds found around a single star and the most rocky planets found in one star’s habitable zone, the range of distances where conditions may be just right to allow the presence of liquid water on a planet’s surface.

Further research has helped us understand the planets’ densities, atmospheres, and more!

his animated image shows an artist's concept of the star TRAPPIST-1, an ultra-cool dwarf, and the seven Earth-size planets orbiting it. TRAPPIST-1 is large and glows bright orange, while the planets are smaller and in shades of cool gray-blue. The image is highly stylized to look like glowing balls sitting on a shiny surface, and neither the sizes nor distances are to scale. The planets closer to TRAPPIST-1 have droplets of water standing on the surface around them, indicating that they may have liquid water. Planets further away have frost around them, indicating that those are more likely to have significant amounts of ice, especially on the side that faces away from the star. Our view pans across the system, from the center outward, and faint tan rings depict the orbits of each planet. The image is watermarked with the text “Illustration” and “Credit: NASA/JPL-Caltech/R. Hurt (IPAC).”

Our eighth astronomical gift is … an (almost) eight-foot mirror

The primary mirror on our Nancy Grace Roman Space Telescope is approximately eight feet in diameter, similar to our Hubble Space Telescope. But Roman can survey large regions of the sky over 1,000 times faster, allowing it to hunt for thousands of exoplanets and measure light from a billion galaxies.

Side profile of a man standing in front of the Nancy Grace Roman Space Telescope Primary mirror. The man wears a long white coat, hair net, facemask, and glasses. The man is standing to the left of the mirror, and looking at it. The mirror faces the man, so it appears to be looking back at him. The mirror is a flat, smooth, silver disk with a black cylinder protruding from its center. Behind the mirror, a black square houses hardware for the mirror. The image is watermarked “Credit: NASA/Chris Gunn.”

Our ninth astronomical gift is … a kilonova nine days later

In 2017, the National Science Foundation (NSF)’s Laser Interferometer Gravitational-Wave Observatory (LIGO) and European Gravitational Observatory’s Virgo detected gravitational waves from a pair of colliding neutron stars. Less than two seconds later, our telescopes detected a burst of gamma rays from the same event. It was the first time light and gravitational waves were seen from the same cosmic source. But then nine days later, astronomers saw X-ray light produced in jets in the collision’s aftermath. This later emission is called a kilonova, and it helped astronomers understand what the slower-moving material is made of.

This animated illustration shows what happened in the nine days following a neutron star merger known as GW170817, detected on Aug. 17, 2017. In the first part of the animation, a pair of glowing blue neutron stars spiral quickly towards each other and merge with a bright flash. The merger creates gravitational waves (shown as pale arcs rippling out from the center), a near-light-speed jet that produced gamma rays (shown as brown cones and a rapidly-traveling magenta glow erupting from the center of the collision), and a donut-shaped ring of expanding blue debris around the center of the explosion. A variety of colors represent the many wavelengths of light produced by the kilonova, creating violet to blue-white to red bursts at the top and bottom of the collision. In the second part of the animation, we see the collision as it would appear from Earth, looking like a burst of red light in the lower left and a huge umbrella-shaped cascade of blue light in the upper right, representing X-rays.  The image is watermarked with the text “Credit: NASA's Goddard Space Flight Center/CI Lab” and “Illustration.”

Our tenth astronomical gift is … NuSTAR’s ten-meter-long mast

Our NuSTAR X-ray observatory is the first space telescope able to focus on high-energy X-rays. Its ten-meter-long (33 foot) mast, which deployed shortly after launch, puts NuSTAR’s detectors at the perfect distance from its reflective optics to focus X-rays. NuSTAR recently celebrated 10 years since its launch in 2012.

This animation shows an artist’s concept of the NuSTAR X-ray observatory orbiting above the blue marble of Earth and deploying its 10-meter-long (33 foot) mast shortly after launch in 2012. NuSTAR is roughly cylindrical, with a shiny silver covering and a pair of blue solar panels on each of its sides. As we pan around the spacecraft, silver scaffolding extends from inside, separating the ends of the telescope to the right distance to begin observing the universe in X-rays. The image is watermarked with the text “Illustration” and “Credit: Credit: NASA/JPL-Caltech.”

Our eleventh astronomical gift is … eleven days of observations

How long did our Hubble Space Telescope stare at a seemingly empty patch of sky to discover it was full of thousands of faint galaxies? More than 11 days of observations came together to capture this amazing image — that’s about 1 million seconds spread over 400 orbits around Earth!

This animated image zooms into the Hubble Ultra Deep Field, showing how a tiny patch of “empty” sky turned out to contain about 10,000 galaxies. The sequence begins with a starry backdrop, then we begin to zoom into the center of this image. As we travel, larger and brighter objects come into view, including dazzling spiral and elliptical galaxies in reds, oranges, blues, and purples. The image is watermarked with the text “Credit: NASA, G. Bacon and Z. Levay (STScI).”

Our twelfth astronomical gift is … a twelve-kilometer radius

Pulsars are collapsed stellar cores that pack the mass of our Sun into a whirling city-sized ball, compressing matter to its limits. Our NICER telescope aboard the International Space Station helped us precisely measure one called J0030 and found it had a radius of about twelve kilometers — roughly the size of Chicago! This discovery has expanded our understanding of pulsars with the most precise and reliable size measurements of any to date.

In this simulation of a pulsar’s magnetic fields, dozens of thin lines dance around a central gray sphere, which is the collapsed core of a dead massive star. Some of these lines, colored orange, form loops on the surface of the sphere. Others, colored blue, arc away from two spots on the lower half of the sphere and vanish into the black background. The image is watermarked with the text “Simulation” and “Credit: NASA's Goddard Space Flight Center.”

Stay tuned to NASA Universe on Twitter and Facebook to keep up with what’s going on in the cosmos every day. You can learn more about the universe here.

Make sure to follow us on Tumblr for your regular dose of space!

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misscounterfactual - Retrograde Orbit
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